Geodetic Precession in PSR B1534+12

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dc.creatorStairs, I. H.
dc.creatorThorsett, S. E.
dc.creatorTaylor, J. H.
dc.creatorArzoumanian, Z.
dc.date1999-11-11
dc.date1999-11-24
dc.date.accessioned2026-07-07T02:34:20Z
dc.date.available2026-07-07T02:34:20Z
dc.descriptionWe present Arecibo observations of PSR B1534+12 which confirm previous suggestions that the pulse profile is evolving secularly. This effect is similar to that seen in PSR B1913+16, and is almost certainly due to general relativistic precession of the pulsar's spin axis.
dc.description4 pages, 2 figures. Corrected a reference. To appear in proceedings of IAU Colloquium 177: Pulsar Astronomy - 2000 and Beyond
dc.identifierhttps://arxiv.org/abs/astro-ph/9911198
dc.identifierhttp://arxiv.org/abs/astro-ph/9911198
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15206
dc.subjectAstrophysics
dc.titleGeodetic Precession in PSR B1534+12
dc.typetext

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